One Dark Matter Profile Please, Hold the Subhaloes
When we observe galaxies and measure their dark matter halos, we exclude subhaloes from the halo’s mass profile. When we simulate haloes, we include them. But what if we didn’t?
When we observe galaxies and measure their dark matter halos, we exclude subhaloes from the halo’s mass profile. When we simulate haloes, we include them. But what if we didn’t?
New simulations provide insights on the processes behind the formation of massive stars
How do you form Mercury, Venus, Earth AND Mars? The answer may surprise you! (or not ¯\_(ツ)_/¯)
Accounting for the uncertainty in supernova explosion parameters can substantially change the star formation history and morphology of galaxy simulations.
Can a chain reaction in the magnetic field supply the energy to keep the solar atmosphere at a temperature of several million Kelvin?
Today’s undergraduate research post is seeking to automatically identify variable stars in the upcoming all sky survey, LSST. Read on to find out more!